Spectral decomposition of galaxy spectrum at $R=-5\stackrel{″}{.}96$ (upper panel) and $+5\stackrel{″}{.}89$ (lower panel), where the contribution of the counter-rotating component is maximum. The observed spectrum (in the observer-frame, black line) is modeled by the sum (green line) of the contributions of two stellar components, corresponding to the counter-rotating stellar ring (blue line) and host galaxy (red line). The observed spectrum is normalized at its median value. No emission lines are visible in the galaxy spectrum across the entire slit. The artifact at 5577 Å is due to over-subtraction of the O I sky emission line at 5577 Å.